Upper Limits on the Stochastic Gravitational-Wave Background from
Advanced LIGO's First Observing Run

Abbott,; and Abbott, B. P.; and Abbott, R.; and Abernathy, T. D.; and Acernese, M. R.; and Ackley, F.; and Adams, K.; and Adams, C.; and Addesso, T.; and Adhikari, P.; and Adya, R. X.; and Affeldt, V. B.; and Agathos, C.; and Agatsuma, M.; and Aggarwal, K.; and Aguiar, N.; and Aiello, O. D.; and Ain, L.; and Ajith, A.; and Allen, P.; and Allocca, B.; and Altin, A.; and Ananyeva, P. A.; and Anderson, A.; and Anderson, S. B.; and Appert, W. G.; and Arai, S.; and Araya, K.; and Areeda, M. C.; and Arnaud, J. S.; and Arun, N.; and Ascenzi, K. G.; and Ashton, S.; and Ast, G.; and Aston, M.; and Astone, S. M.; and Aufmuth, P.; and Aulbert, P.; and Avila-Alvarez, C.; and Babak, A.; and Bacon, S.; and Bader, P.; and Baker, M. K. M.; and Baldaccini, P. T.; and Ballardin, F.; and Ballmer, G.; and Barayoga, S. W.; and Barclay, J. C.; and Barish, S. E.; and Barker, B. C.; and Barone, D.; and Barr, F.; and Barsotti, B.; and Barsuglia, L.; and Barta, M.; and Bartlett, D.; and Bartos, J.; and Bassiri, I.; and Basti, R.; and Batch, A.; and Baune, J. C.; and Bavigadda, C.; and Bazzan, V.; and Beer, M.; and Bejger, C.; and Belahcene, M.; and Belgin, I.; and Bell, M.; and Berger, A. S.; and Bergmann, B. K.; and Berry, G.; and Bersanetti, C. P. L.; and Bertolini, D.; and Betzwieser, A.; and Bhagwat, J.; and Bhandare, S.; and Bilenko, R.; and Billingsley, I. A.; and Billman, G.; and Birch, C. R.; and Birney, J.; and Birnholtz, R.; and Biscans, O.; and Biscoveanu, S.; and Bisht, A. S.; and Bitossi, A.; and Biwer, M.; and Bizouard, C.; and Blackburn, M. A.; and Blackman, J. K.; and Blair, J.; and Blair, C. D.; and Blair, D. G.; and Bloemen, R. M.; and Bock, S.; and Boer, O.; and Bogaert, M.; and Bohe, G.; and Bondu, A.; and Bonnand, F.; and Boom, R.; and Bork, B. A.; and Boschi, R.; and Bose, V.; and Bouffanais, S.; and Bozzi, Y.; and Bradaschia, A.; and Brady, C.; and Braginsky, P. R.; and Branchesi, V. B.; and Brau, M.; and Briant, J. E.; and Brillet, T.; and Brinkmann, A.; and Brisson, M.; and Brockill, V.; and Broida, P.; and Brooks, J. E.; and Brown, A. F.; and Brown, D. A.; and Brown, D. D.; and Brunett, N. M.; and Buchanan, S.; and Buikema, C. C.; and Bulik, A.; and Bulten, T.; and Buonanno, H. J.; and Buskulic, A.; and Buy, D.; and Byer, C.; and Cabero, R. L.; and Cadonati, M.; and Cagnoli, L.; and Cahillane, G.; and Bustillo, C.; Calderon and Callister, J.; and Calloni, T. A.; and Camp, E.; and Campbell, J. B.; and Canepa, W.; and Cannon, M.; and Cao, K. C.; and Cao, H.; and Capano, J.; and Capocasa, C. D.; and Carbognani, E.; and Caride, F.; and Diaz, S.; Casanueva and Casentini, J.; and Caudill, C.; and Cavaglia, S.; and Cavalier, M.; and Cavalieri, F.; and Cella, R.; and Cepeda, G.; and Baiardi, C. B.; Cerboni and Cerretani, L.; and Cesarini, G.; and Chamberlin, E.; and Chan, S. J.; and Chao, M.; and Charlton, S.; and Chassande-Mottin, P.; and Cheeseboro, E.; and Chen, B. D.; and Chen, H. Y.; and Cheng, Y.; and Chincarini, H. -. P.; and Chiummo, A.; and Chmiel, A.; and Cho, T.; and Cho, H. S.; and Chow, M.; and Christensen, J. H.; and Chu, N.; and Chua, Q.; and Chua, A. J. K.; and Chung, S.; and Ciani, S.; and Clara, G.; and Clark, F.; and Cleva, J. A.; and Cocchieri, F.; and Coccia, C.; and Cohadon, E.; and Colla, P. -. F.; and Collette, A.; and Cominsky, C. G.; and Constancio, L.; J. r.,; and Conti, M.; and Cooper, L.; and Corbitt, S. J.; and Cornish, T. R.; and Corsi, N.; and Cortese, A.; and Costa, S.; and Coughlin, C. A.; and Coughlin, E.; and Coughlin, M. W.; and Coulon, S. B.; and Countryman, J. -. P.; and Couvares, S. T.; and Covas, P.; and Cowan, P. B.; and Coward, E. E.; and Cowart, D. M.; and Coyne, M. J.; and Coyne, D. C.; and Creighton, R.; and Creighton, J. D. 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doi:10.1103/PhysRevLett.118.121101

A wide variety of astrophysical and cosmological sources are expected to contribute to a stochastic gravitational-wave background. Following the observations of GW150914 and GW151226, the rate and mass of coalescing binary black holes appear to be greater than many previous expectations. As a result, the stochastic background from unresolved compact binary coalescences is expected to be particularly loud. We perform a search for the isotropic stochastic gravitational-wave background using data from Advanced Laser Interferometer Gravitational Wave Observatory's (aLIGO) first observing run. The data display no evidence of a stochastic gravitational-wave signal. We constrain the dimensionless energy density of gravitational waves to be Omega(0) < 1.7 x 10(-7) with 95\% confidence, assuming a flat energy density spectrum in the most sensitive part of the LIGO band (20-86 Hz). This is a factor of similar to 33 times more sensitive than previous measurements. We also constrain arbitrary power-law spectra. Finally, we investigate the implications of this search for the background of binary black holes using an astrophysical model for the background.

Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run

Abbott;B. P. and Abbott;R. and Abbott;T. D. and Abernathy;M. R. and Acernese;F. and Ackley;K. and Adams;C. and Adams;T. and Addesso;P. and Adhikari;R. X. and Adya;V. B. and Affeldt;C. and Agathos;M. and Agatsuma;K. and Aggarwal;N. and Aguiar;O. D. and Aiello;L. and Ain;A. and Ajith;P. and Allen;B. and Allocca;A. and Altin;P. A. and Ananyeva;A. and Anderson;S. B. and Anderson;W. G. and Appert;S. and Arai;K. and Araya;M. C. and Areeda;J. S. and Arnaud;N. and Arun;K. G. and Ascenzi;S. and Ashton;G. and Ast;M. and Aston;S. M. and Astone;P. and Aufmuth;P. and Aulbert;C. and Avila-Alvarez;A. and Babak;S. and Bacon;P. and Bader;M. K. M. and Baker;P. T. and Baldaccini;F. and Ballardin;G. and Ballmer;S. W. and Barayoga;J. C. and Barclay;S. E. and Barish;B. C. and Barker;D. and Barone;F. and Barr;B. and Barsotti;L. and Barsuglia;M. and Barta;D. and Bartlett;J. and Bartos;I. and Bassiri;R. and Basti;A. and Batch;J. C. and Baune;C. and Bavigadda;V. and Bazzan;M. and Beer;C. and Bejger;M. and Belahcene;I. and Belgin;M. and Bell;A. S. and Berger;B. K. and Bergmann;G. and Berry;C. P. L. and Bersanetti;D. and Bertolini;A. and Betzwieser;J. and Bhagwat;S. and Bhandare;R. and Bilenko;I. A. and Billingsley;G. and Billman;C. R. and Birch;J. and Birney;R. and Birnholtz;O. and Biscans;S. and Biscoveanu;A. S. and Bisht;A. and Bitossi;M. and Biwer;C. and Bizouard;M. A. and Blackburn;J. K. and Blackman;J. and Blair;C. D. and Blair;D. G. and Blair;R. M. and Bloemen;S. and Bock;O. and Boer;M. and Bogaert;G. and Bohe;A. and Bondu;F. and Bonnand;R. and Boom;B. A. and Bork;R. and Boschi;V. and Bose;S. and Bouffanais;Y. and Bozzi;A. and Bradaschia;C. and Brady;P. R. and Braginsky;V. B. and Branchesi;M. and Brau;J. E. and Briant;T. and Brillet;A. and Brinkmann;M. and Brisson;V. and Brockill;P. and Broida;J. E. and Brooks;A. F. and Brown;D. A. and Brown;D. D. and Brown;N. M. and Brunett;S. and Buchanan;C. 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J. and Yu;Hang and Yu;Haocun and Yvert;M. and Zadrozny;A. and Zangrando;L. and Zanolin;M. and Zendri;J. -.P. and Zevin;M. and Zhang;L. and Zhang;M. and Zhang;T. and Zhang;Y. and Zhao;C. and Zhou;M. and Zhou;Z. and Zhu;S. J. and Zhu;X. J. and Zucker;M. E. and Zweizig;

2017-01-01

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	Anno di pubblicazione
	
				2017
			
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				PHYSICAL REVIEW LETTERS
			
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				https://dx.doi.org/10.1103/PhysRevLett.118.121101
			
	ID tipologia loginMiur
	
				262
			
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11581/405212

Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run

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Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run

2017-01-01

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